The Nature Of X-Ray Emission In Nearby Dwarf Galaxies: The Case Of NGC 625

Details The Nature Of X-Ray Emission In Nearby Dwarf Galaxies: The Case Of NGC 625 The Nature Of X-Ray Emission In Nearby Dwarf Galaxies: The Case Of NGC 625

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1496s&link_type=abstract

Chandra Proposal ID #05600329

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Chandra Proposal Id #05600329

Scientific paper

We propose to add a 60 ksec ACIS-S observation to a multi-wavelength (XMM, FUSE, HST, CTIO, JCMT, ATCA) study of NGC 625, a nearby dwarf starburst galaxy showing coincident diffuse X-ray and H-alpha emission indicative of an active outflow from the starburst region. Chandra observations will allow us to isolate point sources and determine the distribution and temperature of the diffuse X-ray emission. We can then study the energetics of the X-ray superbubble and compare NGC 625 with the few other well-studied low-mass systems harboring active galactic winds, furthering our understanding of the impact of star formation on galaxy evolution.

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